Sugars detected in interstellar space

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Future astronauts won't need to worry about their tan in space, as international researchers have detected sugars in space that we commonly find in sunless tanning cosmetics (as well as raspberries). This sugar, called erythrulose, is made up of four carbon atoms and has been detected near the centre of our Milky Way galaxy, say the team. The astronomers pointed a pair of radio telescopes at a large cloud of dust in interstellar space and identified the sugar by matching the signal to the pattern for erythrulose that they measured in the laboratory. The team say erythrulose was at least eight times more abundant in the cloud than other sugars with one fewer carbon atom; these, however, were not detected in the same location.

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From: Springer Nature

A type of sugar made of four carbon atoms, called erythrulose, has been identified near the centre of the Milky Way galaxy, according to research published in Nature Astronomy. This finding indicates that complex, biologically relevant molecules can form in space and may contribute to the chemical ingredients available for early metabolic and replication processes.

Sugars are important molecules in living systems, helping to provide energy, build important biological structures, and form parts of genetic material. On Earth, erythrulose is commonly found in raspberries and sunless tanning cosmetics. Scientists have long wondered how these molecules first formed on Earth, because experiments show they do not easily form under early Earth conditions. The previous discovery of ribose and glucose in meteorite and asteroid samples has suggested that some sugars may have come from space, but until now, no sugar had been directly detected in the interstellar medium.

Izaskun Jiménez-Serra and colleagues report the detection of erythrulose in a large cloud of gas and dust called G+0.693-0.027, located near the centre of the Milky Way galaxy. They observed the cloud with the Yebes 40-metre and IRAM 30-metre radio telescopes in Spain. The authors identified the sugar by matching signals in the data to the pattern for erythrulose measured in the laboratory, finding 12 matching sets. They also found that erythrulose is at least eight times more abundant in the gas cloud than similar sugars with three carbon atoms, which were not detected in the same location.

The findings suggest that erythrulose can be made from simpler molecules on dust grains in space and may then become part of more complex chemical systems.

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Nature Astronomy
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Organisation/s: CSIC-INTA, Torrejón de Ardoz, Spain
Funder: This work is supported by ERC grant OPENS, GA no. 101125858 funded by the European Union. Views and opinions expressed are, however, those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council Executive Agency. Neither the European Union nor the granting authority can be held responsible for them. I.J-.S., J.G.d.l.C., M.S.-N., V.M.R., J.M.-P., L.C., S.Z., S.M., A.M., A.M.-H., A.L.-G., M.A.R.-T. and D.S.A. also acknowledge partial support from grant number PID2022-136814NB-I00 funded by the Spanish Ministry of Science, Innovation and Universities/State Agency of Research MICIU/AEI/ 10.13039/501100011033 and by ‘ERDF/EU’. I.J-.S., A.M. and S.Z. acknowledge partial support from the CSIC Bilateral project SOULMATE (BIJSP25017). J.G.d.l.C. acknowledges support from European Funds for Regional Development and the Autonomous Government of Extremadura (grant no. GR24020). M.S.-N. also acknowledges a Juan de la Cierva Postdoctoral Fellowship, project JDC2022-048934-I, funded by MCIN/AEI/10.13039/501100011033 and by the European Union ‘NextGenerationEU/PRTR’, and a Humboldt Research Fellowship funded by the Alexander von Humboldt foundation. V.M.R. aknowledges support through grant RYC2020-029387-I funded by MICIU/AEI/10.13039/501100011033 and by ‘ESF, Investing in your future’, and from the Consejo Superior de Investigaciones Científicas (CSIC) and the Centro de Astrobiología (CAB) through the project 20225AT015 (Proyectos intramurales especiales del CSIC). V.M.R. and D.S.A. acknowledge support from grant CNS2023-144464 funded by MICIU/AEI/10.13039/501100011033 and by ‘European Union NextGenerationEU/PRTR’. D.S.A. acknowledges the financial support provided by the Comunidad de Madrid through the grant PIPF-2022/TEC-25475. L.C. acknowledges support from a research fellowship from the ‘la Caixa’ Foundation (ID 100010434 – fellowship code LCF/BQ/ PR25/12110012). B.T. acknowledges Spanish Ministry of Science support from grants PID2022-137980NB-100 and PID2023- 147545NB-I00. A.L-G. and D.S.A acknowledge support from the Consejo Superior de Investigaciones Científicas (CSIC) and the Centro de Astrobiología (CAB) through the project 20225AT015 (Proyectos intramurales especiales del CSIC). E.J.C. acknowledges support from the Basque Government (project IT1491-22) and from grant PID2023-147698NB-I00 funded by MCIN/AEI/10.13039/501100011033 and ERDF/EU, and the CSIC I-LINK project ILINK25125.
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